Abstract
The results on the solar neutrino measurement covering over 7 years in the Kamiokande detector are explained, and their systematic errors are briefly reviewed. The time averaged flux assuming the shape of the 8 B beta decay is (2.89 −0.21 +0.22 ±0.35) × 10 6 cm 2 / sec and the ratio of the flux to the standard solar model of Bahcall and Pinsonnault is 0.51 ± 0.04 ± 0.06. Model independent approaches to the solar neutrino problem that we can conduct by the future solar neutrino experiment, Superkamiokande, are also presented.
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